Processing of multiple wavelength signals transmitted through free space

ABSTRACT

The present invention is directed to a laser communication receiver for wireless optical communication. A laser communication receiver includes a diffractive optical element to permit detectors at different spatial locations to detect different wavelengths of the optical signal. An immersion lens may be employed to focus the optical signal to a spot size smaller than the photoactive area of the detector. In one detector configuration, the optical signal is folded by a reflective surface and focused on a plurality of stacked detectors. The present invention further provides a method of manufacturing a detector and immersion lens assembly that provides a high degree of alignment between the lens and the corresponding detector.

CROSS REFERENCE TO RELATED APPLICATIONS

The present application claims under 35 U.S.C.§119(e) the benefits of U.S. Provisional Application Ser. No. 60/264,079, filed Jan. 24, 2001, entitled “On Axis Laser Receiver Wavelength Demultiplexer with Integral Immersion Lensed Detectors” and is under 35 U.S.C.§120 a continuation-in-part of U.S. patent application Ser. No. 09/339,316, filed Jun. 23, 1999, to Smith entitled “RECEIVING MULTIPLE WAVELENGTHS AT HIGH TRANSMISSION RATES”, both of which are incorporated herein by this reference.

FIELD OF THE INVENTION

The present invention relates to laser communication receivers, and more specifically to an apparatus and method to receive high data rate signals transmitted through free space.

BACKGROUND INFORMATION

Various communication systems are known for transmitting through the atmosphere. Most commonly, microwave communication devices are used for this communication. Additionally, various optical techniques for communication are known.

Microwave technologies used for data links through the atmosphere generally suffer from low data rates. For example, an 11 to 14 or 20 to 30 gigahertz (GHz) carrier is sometimes used to transmit between a satellite and a ground station. However, modulating 1 gigabit/sec. data rates on the 18 GHz carrier is not currently practically accomplished. By increasing the carrier frequency, the data rate may also be increased. For example, a 60 GHz carrier could support modulation data rates of 1 gigabit/sec. or higher. However, the atmosphere itself attenuates the 60 GHz carrier such that transmission through the atmosphere is not practical.

Terrestrial-based, free-space optical (laser) transmission systems are being considered as a replacement for free space microwave communications systems. Laser systems generally enable data to travel between a ground-based transmitter and a ground-based receiver at high rates a data rates. In laser communication systems, an optical carrier is modulated with data to transmit information through the atmosphere. Adaptive optic subsystems may be used to focus the light on a receiver, thereby improving beam quality. The focused light can be collected into a single mode or multimode optical fiber and transmitted via the optical fiber to a de-multiplexing element.

Although laser systems can realize high data transmission rates, they can have significant drawbacks.

For example, conventional non-diffractive telescopes focus not only the optical signal but also sunlight onto other optical components. This can cause significant damage to the components, saturate the system, or introduce noise into the optical signal, causing higher bit error rates (BER).

Laser receivers can demultiplex different wavelength bands within the received power that is converging to a focus from the primary optical lens. Such demultiplexing typically requires recollimation of the received beam, reflecting the beam off a line-of-sight stabilization mirror, routing through an optical fiber, collimation after passage via the fiber to a series of bandpass filters, each of which diverts a particular wavelength to an exit lens and fiber for routing to a detector unit. This cumbersome configuration can suffer from significant optical losses, is tedious, and costly. Laser systems typically require the transmit and/or receive telescopes to be large (e.g., have an aperture of more than 20 inches) and therefore expensive. By way of example, when a telescope's aperture size is increased from 10 to 20 inches the cost also increases by a factor of 5 or 6. The need to collect the light onto the optical fiber introduces additional size and expense. The fiber can normally only receive light that is within a 30° cone, which, for a large receive aperture, requires a long optical path from the telescope to the fiber.

Laser receivers can have high BERs. BERs can be increased by the effects of atmospheric turbulence. The effects of atmospheric disturbances from thermal air currents along the optical path are typically greatest at the transmitter and receiver. For a terrestrial link, the transmitter and receiver are typically (compared to other parts of the optical path) in closest proximity to thermal sources, namely solid surfaces such as the ground and rooftops, which absorb solar flux and warm the air. The warm air rises through cooler air thereby generating turbulence and providing a non-uniform propagation medium for the optical signal. At the transmitter, such disturbances can cause different portions of the optical beam to pass through differently moving air currents, causing the propagating beam to break up, so leaving the receive aperture in an intensity minimum. Similar disturbances near the receive aperture can cause the focal spot to break up, leaving the detector in an intensity minimum. Each of these distinct processes can produce burst errors in the communicated data and must be addressed separately. As will be appreciated, a burst error refers to a period of optical extinction. The focal spot of the optical beam can be smeared. If the received optical signal power has passed through air, atmospheric turbulence will inevitably smear out the focal spot somewhat relative to the desired focal spot diameter. Imperfections in the primary optical lens can also smear out the focal spot. Since only small detectors, e.g., 60 microns in diameter, are able to respond fast enough to resolve temporarily the 400 picosecond pulses of wideband, e.g., 2.5 Gbps, data streams, the efficiency of any such detector is downgraded by its inability to collect all the power in the focal spot.

SUMMARY OF THE INVENTION

In accordance with the present invention, apparatuses and methods for high-bandwidth wireless data transmission, particularly through the atmosphere, are disclosed.

In a first embodiment, a primary optical lens that is a diffractive optical element, such as a transmissive or reflective hologram, zone plate, etc., receive radiation of one or more wavelengths that has been modulated by high frequency data. As will be appreciated, a diffractive optical element spatially separates different wavelengths of radiation or wavelength bands, preferably focusing each wavelength or wavelength band of radiation to a different spatial location. A detector assembly, that is responsive to the respective focused radiation, is preferably positioned at or near each focal area or point. Each detector assembly detects the data in the respective beam focused on the detector assembly. In one configuration, the detector assemblies are in a stacked or end-to-end configuration and are located along a common axis, which can be the optical axis of the primary optical lens.

This receiver configuration can realize high data transmission rates through free space without the drawbacks associated with conventional telescope receivers. As used herein, “transmission through free space” and “free space transmission” refers to a beam of radiation traversing an optical path, at least a portion of which is free of a waveguide, such as an optical fiber. Free space transmission, for example, includes transmission of radiation through the earth's atmosphere such as between two earth-based stations or between an earth-based and space-based station and through space such as between two space-based stations. The receiver of the present invention can be much less inexpensive and smaller than conventional telescope receivers, and operated for long intervals of time and during daylight without damaging optical components in the receiver.

The laser communication receiver differs from previous methods of wavelength demultiplexing in that the present invention need not collimate, repoint and reroute to a separate demultiplexer signal power that is converging to a focus from the primary optical lens. The detector units of the laser communication receiver of the present invention are in the converging beam of the primary optical lens. Since a diffractive optical element focuses different wavelengths to different on-axis locations, placement of detector units at these on-axis locations results in channel separation. The primary optical lens focuses at least most of the sunlight beyond the detector units if at all. Only that portion, if any, of the sunlight having the proper wavelength can be focused on each detector assembly.

In another embodiment, the detector assembly for a laser communication receiver includes a focusing element (in addition to the diffractive optical element) to reduce further the spot size of the radiation focused on the detector assembly. The focusing element can be any lens that further decreases the spot size of the radiation. Examples of such focusing elements include a solid immersion lens (SIL), and an oil immersion lens. The detector is typically in physical contact with or “immersed” in the focusing element.

The additional focusing element is particularly effective in accounting for the detrimental effect of atmospheric turbulence, lens imperfections, and window imperfections on data transmission. The focusing element increases detector efficiency by reducing the spot size of the focused radiation to a size smaller than the size of the photoactive area of the detector unit. The small spot size reduces the adverse effect of atmospheric turbulence and lens imperfections on data transmission. The focusing element averages out such adverse effects by permitting the detector unit to collect a greater amount of the radiation contacting the receiver aperture than has previously been possible. This feature thus provides a more robust laser communication receiver.

The aperture size of the receiver preferably is larger than the Fresnel scale. Because atmospheric turbulence is a common phenomenon, destructive interference is typically present in some portion of the beam incident on the receiver. If not bigger than the Fresnel scale (i.e., given as √{square root over (λ·Z)}, where λ=propagation wavelength and Z=propagation distance), the receiver aperture can encounter periods where the entire subtended optical signal is nonexistent due to turbulence far from the receiver.

In yet another embodiment, a laser communication receiver, that is particularly useful for free space transmission, includes a reflective surface for reflecting the focused optical signal onto a detector positioned to receive the reflected radiation. The reflective surface can be any suitable reflecting optical element such as a full or partial silvered mirror. In one configuration, a number of detector assemblies are positioned in a hole of the primary optical lens and the reflective or refractive surface is positioned on a first side of the lens where the radiation is focused. The optical path is folded back on itself such that the direction of the reflected optical path is at least substantially parallel to the incoming optical path direction. In this configuration, some of the detector assemblies can be located on the opposite second side and/or on the first side of the lens. This receiver configuration has a shallow depth and is compact and robust in design.

Another embodiment provides a method of manufacturing a detector assembly. The optical detector unit is formed on an at least substantially transparent substrate and a curved (or spherical or essentially hemispherical) surface (or SIL) is formed on the other side of the substrate. As noted above, the curved surface focuses the radiation onto the detector unit and thereby reduces the spot size of the incoming radiation.

This method has a number of benefits. An SIL is typically small, e.g., about 200 microns diameter, if it is to collect the smeared out power. Such a small lens is difficult to align to an approximately 60 micron detector unit, particularly when optical contact typically requires a spring-loaded assembly and wire bond attachment points are in locations where they impede the optical contact. Making the SIL an integral part of the detector can eliminate these alignment problems.

In yet another embodiment, the laser receiver is synergistically combined with a laser communication transmitter is provided that emits a beam having a smaller diameter than the inner scale as measured at the transmitter aperture to realize unexpected benefits. Such beams can substantially minimize power fades from atmospheric turbulence and therefore the occurrence of burst errors. As used herein, “inner scale” refers to the smallest distance across which an air temperature difference can be sustained. Because the critical first few meters of especially strong turbulence are within the Rayleigh range

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$\left( {{i.e.},\mspace{14mu}{{given}\mspace{14mu}{by}\mspace{14mu}\frac{({beamdiameter})^{2}}{1.27\lambda}}} \right),$ the beam diameter is kept so small as to see only minimal refractive index variation across its diameter and thereby avoids the wavefront distortions which could have Fourier-transformed to an interference pattern in the far-field. The beam thus inhibits large area destructive interference near the receive aperture. The far-field divergence angle is large enough (typically from about 0.1 to about 2.0 milliradians and more typically from about 0.4 to about 1.0 milliradian) that it cannot be steered off the receiver by the turbulent air. The bigger far-field divergence angle reduces the interference of portions of the beam beyond its Rayleigh range, by virture of their divergent Poynting vectors. In one configuration, a relatively large, low quality laser communication receiver aperture (i.e., photon bucket), typically on the order of at least about 0.2m and more typically about 0.4m, can then adjust for the big transmit divergence by subtending a large solid angle from the transmitter. The larger aperture captures enough of the radiation to compensate for the lower intensity radiation from the purposely broadened transmit beam.

The laser transmitter and laser receiver described above can provide low bit error rates for a given set of atmospheric conditions. Typically, the bit error rate is no more than about 1×10⁻⁹ and even more typically no more than about 1×10⁻¹². This is much lower than the typical minimum achievable bit error rate in most applications, which is approximately 1×10⁻⁶.

Additional advantages of the present invention will become readily apparent from the following discussion, particularly when taken together with the accompanying drawings.

BRIEF DESCRIPTION OF THE DRAWINGS

FIG. 1 is a block diagram of a laser communication system which communicates at high data rates through the atmosphere;

FIG. 2 depicts a technique for reducing the adverse effect of the atmospheric turbulence at the transmitter aperture;

FIG. 3 depicts the relationship between divergence angle and the optical receiver;

FIG. 4 depicts a technique for positioning the optical receiver aperture relative to the divergent optical signal;

FIG. 5 is a schematic view of an optical receiver according to an embodiment of the present invention;

FIG. 6A is a schematic view of focal cones for different wavelength radiation being focused by a reflective hologram; and

FIG. 6B is a schematic view of two focal cones for differing wavelength radiation being focused by a transmissive hologram;

FIG. 7 is a schematic view of an optical detector assembly according to an embodiment of the present invention;

FIG. 8 is a perspective view of a transmissive holographic unit according to an embodiment of the present invention;

FIG. 9 is a perspective view of an optical receiver according to an embodiment of the present invention;

FIG. 10 is a cross-sectional view along line 10—10 of the optical receiver of FIG. 9;

FIG. 11 is a perspective view of a detector barrel for a six channel optical receiver;

FIG. 12 is a cross-sectional view taken along line 12—12 of the detector barrel of FIG. 11;

FIG. 13 is a front view of a detector assembly according to an embodiment of the present invention;

FIG. 14 is a plan view of a substrate including a plurality of detector units and a corresponding plurality of lenses or essentially hemispherical surfaces;

FIG. 15 is a cross-sectional view of a detector unit and immersion lens according to another embodiment of the present invention; and

FIG. 16 is a schematic view of an optical receiver according to yet another embodiment of the present invention.

DETAILED DESCRIPTION

The architecture of the present invention controls the detrimental effects of atmospheric turbulence at the transmitter by using a beam having a smaller diameter than the inner scale as measured at the transmit aperture and/or that is divergent and/or broad and/or a receive aperture that exceeds the Fresnel scale (to average out any smaller diameter intensity variations (within the beam footprint)). The use a smaller diameter beam has a significantly reduced likelihood of passing through differently moving air currents and thereby experiencing break up. The use of the divergent beam reduces the likelihood that the beam footprint will wander off of the receive aperture. As will be appreciated, a collimated beam of diameter “d” and wavelength “w” maintains its diameter for the Rayleigh range. After the Rayleigh range, the collimated beam diverges at an angle defined by w/d. The diverging beam diameter at any distance “z” from the transmitter (but beyond the Rayleigh range) is referred to as the footprint of the beam and is defined by wz/d.

The architecture controls the detrimental effects of atmospheric turbulence at the receiver by using a diffractive optical element to provide a plurality of converging optical signals (having spatially offset focal points) corresponding to differing optical wavelengths and/or an immersed detector to at least substantially maximize the optical signal power received by the detector. An essentially hemispherical immersion lens is positioned between the diffractive optical element and the detector to increase substantially the irradiance of the optical signal on the photoactive area of the detector.

With reference to FIG. 1, a simplex embodiment of a laser communication system 100 is shown in block diagram form. The laser communication system 100 includes a laser communication transmitter 104 and a laser communication receiver 102. As will be appreciated, a duplex system may be implemented by placing a transmitter and receiver at each end of the link.

The Laser Communication Transmitter

The laser communication transmitter 104 can include one or a number of optical transmitters 132. The optical transmitters 132 each transmit a modulated laser beam 112 having a different wavelength λ. In one embodiment, there are four modulated laser beams 112 having wavelengths near 1550 nanometers where each wavelength differs by approximately 4 nanometers. Each laser beam 112 has a footprint which is increased by the atmospheric distortion 108. The footprint is a cross-sectional diameter of the laser beam 112 at the receive terminal focal plane 106. Data is modulated in one or more of intensity, frequency, and phase onto a laser light carrier and is demodulated later from the laser light carrier in order to transport data great distances. The present embodiment assumes that intensity modulation of the transmit laser is used. In the laser communication transmitter, an optical transmitter 132 modulates data on a laser light carrier to form a modulated laser beam 112. The laser beam 112 is modulated with data at a rate greater than about 1 gigabit/sec. and preferably, greater than about 2 gigabit/sec. In order for the laser beam 112 to reach the laser communication receiver 102, the beam 112 travels through atmospheric turbulence 108.

The atmospheric turbulence 108 along the transmission path causes wavefront distortion in modulated laser beams 112. In other words, atmospheric turbulence 108 from thermal currents bends the collimated or diverging laser beams 112 and/or fragments the beam, thereby causing mutual interference or cancellation and so produces burst errors in the data stream.

To overcome or reduce the effect of atmospheric distortion 108 on the bit error rate (BER), the diameter of each of the modulated laser beams 112 at the point 133 (FIG. 2) at which each beam exits its corresponding transmitter 132 (or the aperture of the transmitter) is preferably selected such that the diameter is less than the inner scale of the atmospheric turbulence (or thermal currents) at the respective exit point.

As will be appreciated, the inner scale is typically a function of the temperature of any adjacent thermally conductive surface(s), the ambient air temperature, the distance from the transmit aperture to the adjacent surface(s) and wind speed. The inner scale is commonly from about 5 to about 20% of the distance “D_(T)” (FIG. 2) from the adjacent surface 137 from which the thermal currents are emanating. For example, if the aperture of the transmitter is located at a distance D_(T) of 200 mm above a rooftop, the inner scale would be around 20 mm. Generally, it is desirable to position the transmitter aperture far enough from an adjacent heat absorbing surface such that the inner scale is at least about 20 mm.

In selecting the desired diameter for the beam at the transmit aperture, it is preferable to select the worst case for the particular location and environment in which the transmitter aperture is to be positioned. A suitable safety factor can then be applied to the inner scale and/or beam diameter or the beam diameter otherwise reduced to provide a beam diameter which will be safely below the inner scale under “worst case” conditions. Typically, the diameter of the (Gaussian) transmit beam 112 is no more than about 12.5 mm, more typically it ranges from about 1 to about 10 mm, and even more typically from about 2 to about 5 mm.

As will be appreciated, the beam diameter selection for each of the beams 112 is made independently. Each of the beams 112 could have a different diameter depending upon the magnitude of the inner scale at the point at which the beam 112 exits the corresponding optical transmitter 132.

The divergence angle of the broad beam is selected preferably by determining the “worst case” atmospheric induced deviation of the beam along the beam path and selecting the divergence angle of the beam (FIG. 3) to exceed the turbulence-induced beam deviation for the beam under the worst case conditions. A suitable safety factor can be applied to the divergence angle, as desired. The divergence angle causes the far-field footprint of the beam 112 to remain on the receiver aperture despite atmospheric turbulence. Accordingly, beam 112 should be aimed properly at the receiver even when the beam is subjected to substantial deviation due to atmospheric turbulence 108. Typically, the divergence angle is at least about 20 μr but needs be no more than about 2000 μr and more typically ranges from about 50 μr to about 1000 μr.

To provide further assurance that the far-field footprint of the beam remains on the face of the receiver, the receiver should be oriented properly relative to the incoming beam 112. Referring to FIG. 4, the aperture 116 of the laser communication receiver 102 is preferably positioned/sized relative to the laser communication transmitter 104 such that the receiver 102 subtends at least about 20 μr and more preferably at least about 50 μr of the diverging transmit beam 112 (as shown in FIG. 4).

Although FIG. 1 illustrates a simplex (one-way) system, it is to be understood that the various inventions discussed herein can be used in a full duplex (two-way) system in which one or more transmitters and receivers are positioned at each end of the link.

The Laser Communication Receiver

Referring again to FIG. 1, included in the communication receiver 102 is a holographic unit 116 (or other diffractive optical element), which is a primary optic for the laser communication receiver 102 and a detector assembly 106. The detector assembly 106 includes a focusing element 124 and a detector unit 128 for each modulated laser beam 112. In this embodiment, the transmitter 104 is located in a satellite and the receiver 102 is located in a ground station. However, other embodiments could put the receiver on a building and the transmitter on an airplane (because the receiver benefits are best realized when it is in atmospheric turbulence).

In the laser communication receiver 102, the holographic unit 116 focuses the laser beam 112 into a focus area on a focusing element 124 and detector unit 128. Referring to FIGS. 5, a single holographic unit 116 focuses each laser beam 112 on its respective focusing element 124 and detector unit 128, which is positionally offset (spaced apart) from the other (adjacent) focusing element 124 and detector unit 128. Typically, the distance D_(S) between adjacent detector assemblies 106 a,b ranges from about 1 to about 10 mm with about 2 mm being more typical. As will be appreciated, FIG. 5 is not drawn to scale, with the distance D_(S) being exaggerated relative to the diameter of the diffractive optical element 116. for clarity As can be seen from FIG. 5, the longitudinal axes of the detector units 124 are typically parallel and collinear, and the longitudinal axes of the focusing elements 124 are also typically parallel and collinear. The axes of these components are typically parallel to and collinear with the optical axis 138 of the holographic unit 116. As will be appreciated, the aperture size “A_(S)” of the holographic unit is determined by exceeding the Fresnel scale. By way of example, for a distance between the laser transmitter aperture and laser receiver aperture of 7.25 km and a wavelength of 1.55 microns, the Fresnel scale is √{square root over (7250 m×1.55 μ)}m or 106 mm. The receive aperture is therefore larger than 106 mm and preferably about 400 mm. The modulated laser beams 112 are aimed at the holographic unit 116, whereafter, the laser beams 112 are focused by the holographic unit 116.

The operational differences between reflective and transmissive diffractive optical elements can lead to different receiver configurations. In reflective diffractive optical elements, the focused beam comes from the radiation-receiving side of the element while in transmissive diffractive optical elements the focused beam comes from the opposite side of the element from the radiation-receiving side.

Referring to FIG. 6A, for example, the operation of a reflective hologram 400 is depicted. The reflective hologram 400 focuses radiation 404, 408, corresponding to λ₁ and λ₂ respectively, at differing spacial locations along the optical axis 412 of the hologram. The hologram 400 includes a plurality of concentrically disposed, concave, spherical shells 414 in an emulsion. The locations 418 where the concave spherical shells 414 intersect the hologram surface 424 are spaced inversely with radial position relative to the optical axis 412 of the hologram. This feature ensures that different rings of radiation will phase up to form a cone of light converging to a focus 428, 432 (which correspond respectively to radiation 404 and 408) and that the distance of that focus from the hologram surface 424 will vary inversely with the wavelength of the radiation. For example, the distance of focus 428 from surface 424 is an inverse function of wavelength λ₁, and the distance of focus 432 from surface 424 is an inverse function of wavelength λ₂. A “thick” or “volume” hologram such as that in FIG. 6A has a number of weakly reflecting spherical shells 414 which will cause only radiation for which the spacing of the shells is about one-half of the radiation wavelength to be focused. All other wavelengths of radiation will pass through the hologram. A reflective zone plate would be formed by, for example, evaporating a plurality of concentric silver rings on the plate surface with the spacing between the rings (not shown) varying inversely with the radial position of the ring. The rings would be in the same positions as the ring-shaped intersections between shells 414 and hologram surface 424.

Referring now to FIG. 6B, a transmissive hologram 500 is depicted. The transmissive hologram 500 causes radiation 504 and 508 having wavelengths λ₁ and λ₂, respectively, to focus at different spacial locations 528, 532 along the optical axis 512 of the hologram 500. The transmissive hologram 500 focuses light to the far side of the hologram. The hologram 500 includes a number of annular rings 514 (which appear as a plurality of concentrically disposed rings on hologram surface 524) having a spacing that scales inversely with radial position relative to the optical axis 512. This feature insures that at least some of the concentric rings of radiation passing through the hologram will phase up to create a converging cone of light. The hologram's focal length varies inversely with radiation wavelength. In this manner, all wavelengths shorter than 1.5 microns focus farther from the hologram than does 1.5 microns wavelength. Also, since the annular variations are difficult to reproduce correctly near the optical axis 512 where the spacing is large, the central zone is typically useless. If concentric rings 514 were simply painted onto a flat glass plate, the hologram 500 would be a transmissive zone plate. Alternatively, the rings 514 can be formed by simply etching grooves on the surface. If, as shown, the rings 514 are index ripples and in emulsion, the optical element would be a hologram As will be appreciated, other wavelength bands that are supported by available or developed transmit/receive technologies can also be used with the inventions set forth herein.

Although only holograms are discussed in the detailed description, it is to be expressly understood that any type of diffractive optical element can be employed in place of the holographic unit 116.

Referring again to FIG. 5, the holographic unit 116 is a transmissive hologram that preferably focuses each of the laser beams 112 into a converging cone. Because, as noted above, each laser beam 112 has a different wavelength λ, the focal area (i.e., the tip of the each cone-shaped focus) or focal point is at a different distance from the holographic unit 116. In this embodiment, the focal cone defined by lines 318 a for λ₁ is about 60° to provide good separation between the modulated laser beams 112. Preferably, the focal cone for the various wavelengths ranges from about 30 to about 120° for optimum results.

As will be appreciated, the beams can contact the holographic unit simultaneously or sequentially (at different times), depending on the application. It is also possible for a beam to include multiple wavelengths of radiation, each wavelength representing a different channel and including different transmitted data.

As will be appreciated, the transmissive holographic unit 116 of FIG. 5 has a central obscuration 316 which blocks radiation. As noted, the obscuration is a result of the difficulty in producing the annular variations near the optical axis where the inter-annular variation spacing is large. The obscuration thus creates a shadow. To avoid optical losses, a first detector assembly is located in the shadow of radiation having shorter wavelengths that is detected by detector units positioned behind (or downstream of) the first detector assembly. Referring to FIG. 5 for example, first radiation 318 a of a first (mean or median) wavelength λ₁ is focused on a first focal area 320 a at which a first detector assembly 106 a is positioned. The set of dotted lines 324 a represent the shadow of the central obscuration 316 for the first wavelength radiation but the shadow typically vanishes at the associated detector. Second radiation 318 b of a second (mean or median) wavelength λ is focused on a second focal area 320 b at which a second detector assembly 106 b is positioned. The set of dotted lines 324 b represent the shadow of the central obscuration 316 for the second wavelength radiation. As can be seen, the first detector assembly 106 a is positioned in the shadow of the set of dotted lines 324 b and therefore the first detector assembly 106 a does not cause significant optical losses of the second radiation. This effect can be realized by selecting proper wavelengths of radiation for use in each of the channels, such as for example wavelengths of 1550, 1554, and 1558 nanometers for a three-channel system.

After passing though the atmospheric distortion 108 and being focused by the holographic unit 116, the spot size at the tip of the cone-shaped focus of this embodiment is typically greater than about 100 microns or is approximately 200 microns in diameter. If a 40 micron detector were used with a spot size of 200 microns, only 4% of power would reach the detector. The holographic unit 116 is a passive element and does not allow reshaping of the hologram surface to improve focus. Adaptive optics which allow reshaping of the optics can reduce this spot size with resultant improved focus, but they are expensive and complex.

Referring to FIG. 7, the focusing element 124 overcomes the large focal area of the hologram by receiving the laser beam 112 from the holographic unit 116 and further focusing the light to reduce the spot size diameter. Reducing the spot size allows focusing more light while using a detector diameter small enough for compatibility with high speed transmission on the detector unit 128 which improves data transmission efficiency. The focusing element 124 can be any lens or optical component that increases the irradiance of the focal spot of the radiation. As will be appreciated, light can be focused to a spot whose diameter is inversely proportional to the refractive index of the lens medium 124. For example, a semiconductor immersion lens typically reduces the wavelength of light in air by a factor of about 3 to 4 (i.e., an index of about 3 to 4). In other words, the immersion lens reduces the wavelength of light while within the lens. Preferably, the focusing element increases the intensity of the light by at least a factor of nine. To realize these objectives, the element will typically have an index of refraction of at least about 2.3 and more typically that ranges from about 3.2 to about 4.0. The radius of curvature of the focusing element 124 typically ranges from about 400 to about 600 microns and more typically about 500 microns.

The focusing element 124 typically reduces the spot size of the incident radiation as focused by the holographic unit 116 to a diameter that is less than the photoactive diameter of the detector unit. In an exemplary application, the focusing element 124 reduces to 50 microns the typically greater than about 100 microns and more typically greater than about 200 microns spot size of the beam. Preferably, the spot size is reduced to about 60 microns or less and more preferably to about 40 microns or less. In other words, the spot size of the beam contacting the element 124 is preferably reduced by the focusing element to the photoactive area of the detector unit or less.

The focusing element 124 is preferably one or more of a (solid) immersion lens, and/or an oil immersion lens. Preferably, the focusing element 124 is made of Silicon or Germanium which respectively have indices of refraction of 3.5 and 4 or InP or GaP with indices of refraction near 3.2. Silicon is preferred for wavelengths around 1500 nm and Germanium is preferred for wavelengths around 2000 nm to maximize throughput. Other possible SIL designs that can be employed in the present invention are described in U.S. Pat. No. 6,114,688, which is incorporated herein by this reference.

The focusing element 124 is preferably in physical contact with the detector unit for best results. This physical contacting is known as “immersion”. Immersion can be realized by any suitable technique, such as coaxial alignment and spring force or integral manufacture as discussed below.

The detector unit 128 receives and converts the modulated laser beam 112 into an electrical signal which contains the modulation data. At data rates above 1 gigabit/sec., wide band detectors are required, such as a PIN diode, avalanche photodiode or the like. However, wide band detectors with a large diameter are currently unavailable. As detectors get larger their capacitance increases. If large enough, this capacitance obscures the modulated data. Accordingly, for data rates above 1 gigabit/sec., currently available PIN diodes are generally limited to a diameter of no greater than approximately 60 microns.

Referring to FIG. 8, a transmissive holographic unit 116 according to another embodiment is schematically shown. The holographic unit 116 includes an emulsion layer 300, a flat glass disc 304, and a phase retarder 308.

The phase retarder 308 is any suitable material for altering the phase of the data pulse passing through the phase retarder, e.g., a glass plate. Radiation that contacts the outer peripheral portion of the holographic unit (the area between radii r₁ and r₂) travels a further distance than radiation contacting the central portion of the holographic unit (the area having the outer radii r₁). This delay will cause the portions of the data pulse contacting in these areas to arrive at the detector(s) at different times, leading to smearing of data from differing radiation pulses. The phase retarder 308 causes the data from a given pulse of radiation to arrive at the detector(s) at more nearly the same time. The value of r₁, or the location of the outer periphery 312 of the phase retarder 308, is based upon the desired maximum value of the predetermined time difference. The thickness “t” of the phase retarder typically ranges from about 10 mm to about 30 mm, and r₁ from about 50 to about 80% mm of the hologram radius.

In the absence of the phase retarder, radiation that is focused by peripheral portions of the primary optic will travel a longer distance than radiation that is focused by central portions of the primary optical lens. The different distances traveled can cause data from different pulses to arrive at overlapping times and therefore limit the usable modulation bandwidth. The phase retarder is typically positioned over the central portion of the primary optical lens to cause all portions of the same pulse to arrive within a predetermined time interval of one another and thereby avoid juxtaposition of data from differing pulses.

Referring to FIGS. 9–10, a preferred configuration of a six channel laser communication receiver is depicted. The receiver 600 includes transmissive holographic unit 116, a detector barrel 604 positioned in the central obscuration of the holographic unit 116, frustoconical outer housing 608, reflective surface 612, and phase retarder 308. The detector barrel 604 includes a plurality of detector assemblies 106 a–f, each attached to a transparent substrate 616 a–f; outer cylindrical housing 620, spacer rings 624 a–e positioned between adjacent detector substrates 616 a–f to maintain desired spacings between the detector assemblies 106 a–f, end spacer ring 628 to maintain the rearmost substrate 616 a in the desired position, locating flange 632 to ensure that the detector barrel 604 is mounted and retained in the proper position, and a plurality of coax connectors 636 a–c (six total), each of which corresponds to a separate receive channel. The coax connectors 636 may be attached to a respective detector unit via conductors 640 located along the inner housing wall.

The reflective surface 612, as shown by dotted lines 644, causes incoming radiation to be directed in a reverse direction (or folded back) into the detector barrel. The reflective surface 612 is positioned at a distance “D” from the holographic unit 116 that is approximately equal to one-half of the focal length of the holographic unit 116. In an F/I holographic unit, for example, the distance “D” is one-half of the aperture size of the holographic unit.

As will be appreciated, the reflective surface 612 could be omitted in which case the detector barrel 620 would be located in the base 648 of the housing 608. This design may not be preferred due to the significantly longer length of the housing, which can be problematic in many space restricted applications. The reflective surface can be any suitable reflective optical component, such as a full silvered mirror.

FIGS. 11 and 12 depict a detector barrel 700 according to another embodiment. In contrast to the barrel 604, the barrel 700 includes a cylindrical inner detector ring 704 to position the rearward most detector substrate 616 in position. Spacer rings 620 are used as noted to hold the remaining detector substrates 616 in position. This barrel design further includes a length of a waveguide 708, such as a coax conductor that extends from each coax connector 636 to a respective detector assembly. As will be appreciated, the waveguide could be any other suitable RF interface to post detector electronics. The locating flange 712 is ring-shaped. The interface from the detector assemblies to the next stage of electronics (e.g. amplifier) can be any interface known to one of ordinary skill in the art.

FIG. 13 depicts a preferred design for each detector assembly 106. The detector assembly 106 includes a detector unit 128 positioned on the substrate 616 which is transparent to radiation of the desired optical wavelength (FIG. 10) and which is in the plane of the page. The typically square area 800 is the curved face of immersion lens or focusing element and the round area 804 is the photo active area of the detector unit 128. The width and height of the rectangular immersion lens typically each range from about 100 to about 300 microns and is more typically about 200 microns while the diameter of the round active area 804 typically ranges from about 30 to about 80 microns.

Because of the potential data losses in the conductors from the detector unit to the coax connector 636 at the high data transmission speeds noted above, the conductors are designed according to known transmission line theory. As will be appreciated, the conductors are impedance matched with the detector unit and next stage of the electronics to reduce RF losses. The next stage is most likely an RF interface to a printed circuit board which is followed by an amplifier. The shape of the waveguide typically has stub sections to balance the photodiode impedance and may not be a pure rectangle as shown in the figure. The transmission line can be designed “downward” from the detector unit. The transmission line is preferably a waveguide such as a microstrip or coplanar configuration. In one configuration, a microstrip transmission line 808 extends downwardly from the detector unit 128. The microstrip transmission line 808 includes a conductor 812 and ground plane 816. A first conductive material or “bump” 816, such as indium, attaches to the conductor 812 and a second conductive material or “bump” 820 attaches to the ground plane 816.

The dimensions of the microstrip transmission line 808 depend on the application. Byway of illustration, the ground plane 816 can be about 250 microns in width (“W_(G)”); the conductor 812 about 50 microns in width (“W_(C)”), and the conductor and ground plane separated by about 25 microns (or about 50% of the width of the conductor) of an electrically insulative material, such as a polyimide. The length (“L_(C)) of the conductors depends upon the pulse length of the beam and the impedance of the detector unit and next stage of electronics. For example, if the beam has a pulse length of about 4 inches the length “L_(C)” of the conductors should be less than 10% of the pulse length or less than about 0.4 inches. The cone of radiation 828 converging on the next detector unit is approximately 2 mm in diameter in the plane of the detector unit 128 (or in the plane of the page) and is therefore not blocked to an appreciable extent by the detector unit 128.

Yet another embodiment of a laser communication receiver is shown in FIG. 16. Referring to FIG. 16, a linking device 1200 is placed near the tip of the cone-shaped focus or focal area to redirect the laser beams 112 to their respective focusing element 124. Each laser beam 112 has a focal area which is near its respective linking device 1200. In this embodiment, the linking device 1200 is a pick-off mirror. The pick-off mirror is angled to redirect the laser beam 112 to the focusing element 124.

The detector unit 128 converts the modulated laser beam 112 into an electrical signal which contains the modulation data. At data rates above 1 gigabit/sec., wide band detectors are required, such as a PIN diode or the like. However, wide band detectors with a large diameter are currently unavailable. As detectors get larger their capacitance increases. If large enough, this capacitance obscures the modulated data. Accordingly, for data rates above 1 gigabit/sec., currently available PIN diodes are limited to a diameter of approximately 40 microns.

The focusing element 124 receives the laser beam 112 from the linking device 1200 and focuses the light to reduce the spot size diameter. This focusing preferably reduces to less than 50 microns the greater than 100 micron spot size. Preferably, the spot size is reduced to 40 microns or less. Reducing the spot size allows focusing more light on the detector unit 128 which improves data transmission efficiency. For example, if a 40 micron detector were used with a spot size of 200 microns, only 4% of power would reach the detector.

To enable focusing, the speed of the laser light may be reduced in the focusing element 124 to 30% or less of the speed through free space. The focusing element 124 preferably has an index of refraction of 2 or more. Preferably, the focusing element 124 could be made of Silicon or Germanium which respectively have indices of refraction of 3.5 and 4. Silicon is preferred for wavelengths around 1500 nm and Germanium is preferred for wavelengths around 2000 nm.

With reference to FIG. 16, a channel pick-off assembly or sorter block 2000 is shown with four focal cones 2040 incident thereon. Each focal cone 2040 corresponds to a slightly different wavelength λ and has a focal area 2080 offset from the focal areas 2080 for the other wavelengths λ. The sorter block 2000 includes a glass rod 2120, four linking devices 1200, four focusing elements 124, and four detector units 128. Each focal cone 2040 corresponds to a different modulated laser beam 112 which carries different data. Although not shown in FIG. 16, the holographic unit 116 is positioned so as to produce the four focal cones 2040 which are spaced apart because each results from laser light of slightly different wavelengths λ. Each focal cone 2040 has at its apex a focal area 2080. In this embodiment, the focal cone is 20° to provide good separation between the four modulated laser beams 112.

The linking device, such as pick-off mirror 1200, is positioned at the focal area 2080 to redirect the laser light to a focusing element 124. The pick-off mirrors 1200 are small to reduce the interference with other focal cones 2040. The focusing element 124 focuses the laser light to reduce the spot size for a detector unit 128. Preferably, the detector unit 128 is in direct contact with the focusing element 124, although, it need not be.

The process for manufacturing the detector unit and the focusing element (which further focuses the focal spot of the diffractive optical element) will now be discussed with reference to FIG. 14.

Numerous problems exist in aligning the detector active area and the focusing element using conventional techniques. Traditional techniques of aligning solid immersion lenses with detectors include coaxial alignment and spring force. Traditionally such detectors were on the order of 3 mm in diameter and the immersion lenses of 12 mm in thickness. For acceptable performance in high data rate optical communication, detector sizes are much smaller (e.g., 60 microns) to respond fast enough to temporally resolve the 400 picosecond or shorter pulses of a 2.5 gigabit per second data stream. Not only is it difficult to fabricate the 200 micron solid immersion lens desirable for the 60 micron detectors but also it is difficult to properly orient the lens' axis to that of the much smaller detector unit and subsequently maintain the force needed to produce physical contact without breaking either component. To make matters worse, detector units will typically use a gold wire bond in the electrical connections. These wire bonds are at a minimum 25 microns tall and can interfere with the process of producing physical contact between the SIL and the detector unit unless the back side of the SIL is no larger than the detector unit.

To overcome these problems, a plurality of detector units 1004 are simultaneously formed on a transparent substrate 1000 by known techniques (e.g., epitaxial growth followed by photolithography), the substrate 1000 thereafter thinned, and on the opposite side of the substrate 1000, an essentially hemispherical surface 1008 is aligned and formed opposite to the detector unit 128. Typically, the optical axis of the surface 1008 is aligned (collinear) with and is parallel to the center axis of the corresponding detector unit. In this manner, the alignment and attachment problems encountered with positioning a discrete immersion lens over a detector unit are avoided.

The substrate on which the detector(s) is grown can be any material that is transparent or semitransparent to the desired radiation wavelengths and has the properties referred to above for the focusing element. Preferred substrates include single crystals of indium phosphide, gallium arsenide, or gallium phosphide. Such substrates are transparent to incident signal power in the 1550 nm wavelength band. This combination of properties makes possible the admission of signal from the back (substrate) side through the substrate onto the detector unit.

After growth of the detector crystals 1004 and photolithography, the thickness of the substrate 1000 is typically thinned to the desired diameter of the focal element. For an f/l lens, for example, the appropriate distance for a 200 micron diameter lens is also 200 microns, which is the reduced thickness of the substrate. Typically, the substrate 1000 is thinned to a thickness ranging from about 100 to about 400 microns.

The substrate 1000 is then etched by suitable techniques to form the plurality of focal elements or essentially hemispherical surfaces 1008, each of which is accurately registered or aligned to the location of a corresponding detector. Infrared microscopy can be used to align the mask used to deposit, for example, a photoresist mask on the substrate so that lenses can be wet-etched. Alternatively, the etching can be performed by other techniques such as reactive ion etching, in which an ion beam is directed at individual regions of the substrate for appropriate lengths of time to remove sufficient material to form continuously curved lenses. Another approach is to etch, either by wet process or by reactive ions, Fresnel-type structures as surrogates for the continuously curved lenses, or to approximate the continuous curves by a binary process which produces concentric steps at specific radii and height relative to reference axes. In addition to batch production of immersion lenses and precise coaxial registration of the lenses to a corresponding detector unit, the approach provides the intimate physical contact or detector immersion desired between the lenses and the detector units because they may be both fabricated onto the same substrate.

After batch processing is completed, the lens surfaces are anti-reflection coated. The anti-reflection coating can be any of a number of metal oxides or fluorides.

The substrate is then cleaved by any suitable technique (e.g., or sawed) along horizontal and vertical cut lines 1012, 1016 (which are arranged in a grid pattern) to form a plurality of discrete detector assemblies, each including a substrate, detector unit, and essentially hemispherical surface.

The detector unit can then be “bump” bonded, such as by indium, to another (second) transparent substrate on which the metal conductors have been previously deposited, such as in a microstrip or stripline configuration. Alternatively, the detector unit 128 could be positioned in a hole in the second transparent substrate on which conductors have already been deposited, as shown in FIG. 10.

Another configuration for the detector assembly formed in this manner is shown in FIG. 15. The assembly includes an immersion lens 900 in physical contact with the detector unit 904. A protective coating 908 is formed on the rear surface of the immersion lens 900 and the detector unit 904. Wire bonds 912 connect positive and negative leads 916 and 918 to the detector assembly 106. The immersion lens 900 is, as noted, formed by etching a GaAs or similar substrate on which the detector unit is grown. The detector unit is preferably formed from InGaAs and has a photoactive area ranging from about 30 to about 80 microns in diameter. The diameter of the immersion lens 900 preferably ranges from about 200 to 300 microns.

In this configuration, such coupling through the substrate also avoids another problem of mating SILs to InGaAs-on GaAs detector units—namely the need for the refractive index to remain essentially constant (within a range of about 20% of one another) from the SIL to the detector unit. The reason this is a problem is that fabricators of such detector units typically add a protective coating over the photosensitive InGaAs skin atop the substrate. This protective coating unfortunately has a very low refractive index (typically about 1.5) compared to the SIL (typically about 3.5) and the photosensitive InGaAs skin (typically about 3.5) so the coating degrades passage of signal between the SIL and the InGaAs. By using the GaAs substrate as the SIL, this interface problem disappears. The roughly 200 micron diameter SIL/detector unit would be mounted on transparent substrate or plates 616 (FIG. 13), e.g., microscope slides, which also support transmission lens design for detector output to the electrical preamplifiers (not shown).

The foregoing discussion of the invention has been presented for purposes of illustration and description. Further, the description is not intended to limit the invention to the form disclosed herein. Consequently, variations and modifications commensurate with the above teachings, within the skill and knowledge of the relevant art, are within the scope of the present invention. By way of example only, the invention need not be limited to a hologram as the primary optical element. Any optical element can be used that has zones or areas of varying transmission, reflection, and/or varying refractive index could alternatively be used. The present invention is intended to include other receiver designs not discussed above which would result from using a transmissive and/or reflective diffractive optical element. In the reflective configuration, the detector barrel would be positioned on the laser beam receiving side of the diffractive optical element as the various wavelengths would be reflected by the optical element and received by the spaced apart detectors. Alternatively, the various features noted above can be used separately as part of other transmitter or receiver configurations to realize numerous benefits. For example, the use of a small diameter, so divergent beam can be used with conventional optical receivers to provide significant reductions in burst error occurrence. The optical receiver can be used with a conventional large diameter narrow beam to provide reduced bit error rates. The various elements of the optical receiver can be used in conventional optical receiver designs to further provide enhanced benefits. For example, the use of a larger aperture receiver can provide enhanced benefits. A focusing element, such as the SIL described above, can be used in connection with an otherwise conventional optical receiver to provide reduced fades in the received power. The receiver discussed herein and/or a component thereof may be used in optical communication applications other than free space transmission. By way of example, the receiver and/or component thereof may be used in fiber optic applications, such as a demultiplexer or optical-to-electrical converter. In this application, the receiver would be positioned so as to receive the optical signal transmitted by an optical fiber cable. An optical fiber can be substituted for each detector unit to collect separately each particular wavelength of radiation. An example of such an application is described in U.S. Pat. No. 4,643,519, which is incorporated herein by this reference. Other techniques can be used to produce the focusing element. Examples are discussed in U.S. Pat. Nos. 3,239,675; 4,629,892; 4,636,631; 4,797,179; 5,545,896; and 5,652,813, all of which are incorporated herein by this reference. The detector assembly can be composed of discrete, interconnected components or integrated components. For example, the detector assembly can be an integrated photodetector chip, which would have an amplifier built on the same chip as the PIN detector unit. This design could alleviate some of the engineering problems associated with bleeding off the small RF signal from the detector unit. Because the detector unit feeds a microwave waveguide for some distance before amplification, the signal can pick up additional noise from the other densely packed detector-outputs and other sources (e.g., power supply). The RF signal could be swamped by noise before it reaches the active amplifier. An amplifier and other electronic circuitry for clock and data recovery traditionally follow the detector unit. Alternatively, a MEM (microelectronic mechanism or micromachine) can be integrated into the assembly. MEM's could be applied to a tracking mechanism/feature for orienting/aligning the receiver and emitter. The embodiments discussed hereinabove are further intended to explain the best mode known of practicing the inventions and to enable others skilled in the art to utilize the inventions in such, or in other embodiments and with the various modifications required by their particular application or uses of the inventions. It is intended that the appended claims be construed to include alternative embodiments to the extent permitted by the prior art. 

1. A method for receiving high frequency signals, comprising: transmitting a coherent beam comprising at least one signal including first and second data modulated onto the beam from a laser transmitter through atmospheric turbulence to a receiver, wherein a diameter of the beam comprising said at least one signal is less than an inner scale of an atmosphere at an aperture of said transmitter, wherein a divergence angle of the beam is selected so that it exceeds a determined turbulence induced beam deviation so that a far-field footprint of the beam remains on the receiver aperture despite the atmospheric turbulence, wherein the receiver is located at a distance from the transmitter, wherein the at least one signal, after transmission through the atmospheric turbulence, has a distorted wave-front, wherein said transmitting of said first and second data is conducted at a rate greater than one gigabit/second, and wherein each of said first and second data is associated with first and second wavelength channels, respectively, the first wavelength channel being different from the second wavelength channel; receiving said at least one distorted signal including said first and second data at a detector assembly associated with said receiver; detecting said first data using a first detector unit of the detector assembly, wherein the first detector unit is located at a first position; and detecting said second data using a second detector unit of the detector assembly, wherein the second detector unit is located at a second position that is different from said first position.
 2. A method, as claimed in claim 1, wherein: said detecting first data step includes detecting at the same time, using said first detector unit, all of said first data that was received by said first position of said detector assembly at a particular instance in time.
 3. A method, as claimed in claim 1, wherein: said detecting first data step includes accepting a focal spot size diameter of greater than 40 microns and then reducing said focal spot size diameter.
 4. A method, as claimed in claim 3, wherein: said reducing step includes using a focusing element having a refractive index greater than
 2. 5. A method, as claimed in claim 4, wherein: said focusing element has a traverse length along and through which said first data having said associated first wavelength channel passes, and the speed of said first data in passing along and through said traverse length is no greater than 30% of the speed of light in air.
 6. A method, as claimed in claim 3, wherein: said focal spot size diameter is greater than about 100 microns.
 7. A method, as claimed in claim 1, wherein: said detector assembly includes a linking device, a focusing element and a detector unit.
 8. A method, as claimed in claim 1, further comprising after the transmitting step: finitely focusing, with a holographic unit, said first data to form a first beam and second data to form a second beam.
 9. A method, as claimed in claim 1, wherein: said detecting first data step includes reflecting said first data associated with said first wavelength channel by a first mirror to a focusing element and with an output of said focusing element being in communication with said first detector unit.
 10. A method, as claimed in claim 1, wherein in said receiving step said first data is finitely focused on a first focal point and said second data is finitely focused on a second focal point and the first points is at least substantially at the first location and the second focal point is at least substantially at the second location.
 11. A method, as claimed in claim 1, wherein: said detecting said second data step includes accepting said second data using a linking device, directing said second data to a second focusing element and with the output of said second focusing element being in communication with said second detector unit.
 12. A method, as claimed in claim 1, wherein said transmitting step includes: modulating said first and second data on a respective light beam to form first and second modulated light beams, respectively, and further comprising: demodulating the detected first and second data.
 13. A method, as claimed in claim 7, wherein a first linking device corresponds to the first detector and a second linking device corresponds to the second detector, wherein the first and second linking devices are in different spatial locations, wherein the first data detecting step comprises: redirecting, with the first linking device, said first data from a first optical path to a transversely oriented second optical path, the second optical path intersecting the first detector unit; and wherein said second data detecting step comprises: redirecting, with the second linking device, said second data from a third optical path to a transversely oriented fourth optical path, the fourth optical path intersecting the second detector unit.
 14. A method, as claimed in claim 1, wherein a spacing between said first and second wavelength channels is about 4 nanometers.
 15. A system for receiving high frequency signals, comprising: a receiver that receives at least one signal including first and second data and comprises a detector assembly; and a transmitter that transmits the at least one signal as a beam having a diameter that is less than an inner scale of an atmosphere at or near a transmitter aperture through atmospheric turbulence to the receiver, wherein the receiver is located at a distance of greater than 100 m from the transmitter, wherein the atmospheric turbulence is determined to be associated with a worst case atmospheric turbulence induced deviation of the beam, wherein a divergence angle of the beam is selected to exceed the atmospheric turbulence induced beam deviation for the beam under the determined worst case conditions, wherein the at least one signal, after transmission through the atmospheric turbulence, has a distorted wavefront, wherein said first and second data are each transmitted at a rate greater than one gigabit/second, wherein said first and second data are respectively associated with first and second wavelength channels, the first wavelength channel being different from the second wavelength channel, and wherein the detector assembly comprises at least a first detector unit located at a first position for detecting said first data, and a second detector unit located at a second position for detecting the second data, the second position being different from said first position.
 16. A system, as claimed in claim 15, wherein: said detector assembly includes a first focusing element that finitely focuses the first data onto the first detector unit, wherein a focal spot size of the first data has a diameter of greater than 40 microns.
 17. A system, as claimed in claim 16, wherein: said focusing element has a refractive index greater than
 2. 18. A system, as claimed in claim 17, wherein: said focusing element has a traverse length along and through which said first data having said associated first wavelength channel passes, and the speed of said first data in passing along and through said traverse length is no greater than 30% of the speed of light in air.
 19. A system, as claimed in claim 17, wherein: said focal spot size diameter is greater than about 100 microns.
 20. A system, as claimed in claim 15, wherein: said detector assembly includes a linking device, a focusing element and a detector unit.
 21. A system, as claimed in claim 15, further comprising: a holographic unit that finitely focuses said first and second data in said at least one distorted signal at the first and second locations.
 22. A system, as claimed in claim 16, wherein the detector assembly comprises: a first mirror that reflects said first data associated with said first wavelength channel onto the focusing element.
 23. A method for receiving high frequency data associated with at least a first wavelength channel, comprising: receiving at a first receiving location said first wavelength channel after the first wavelength channel has passed through atmospheric turbulence and thereby become optically distorted; finitely focusing said received first wavelength channel with a first optical element to form a focused first beam having a focused first spot size, wherein said first focused beam is focused at a first location; further finitely focusing the focused first beam with a second optical element at said first location to form a further focused first beam having a further focused first spot size that is smaller than the focused first spot size, wherein the first and second optical elements are at different spatial locations; detecting at least a portion of the data in the further focused first beam; receiving at said first receiving location a second wave length channel after the second wave length channel has passed through atmospheric turbulence and thereby become optically distorted, wherein said first and second wavelength channels are transmitted as part of a first beam; finitely focusing said received second wavelength channel with said first optical element to form a focused second beam having a focused second spot size, wherein said second focus beam is focused at a second location; further finitely focusing the focused second beam with a third optical element at said second location to form a further focused second beam having a further focused second spot size that is smaller than the focused second spot size, wherein the first and third optical elements are at different spacial locations; detecting at least a portion of the data in the further focused second beam.
 24. A method, as claimed in claim 23, wherein the first optical element is a holographic unit.
 25. A method, as claimed in claim 23, wherein the second optical element is a focusing element having a refractive index greater than
 2. 26. A method, as claimed in claim 23, wherein: said second focusing element reduces said focal spot size from a focal spot size diameter of greater than 100 microns to a focal spot size diameter of less than 50 microns.
 27. A method, as claimed in claim 24, wherein: said holographic unit includes at least one of the following: a volume hologram and a holographic mirror. 